The Sun's shape and brightness
[Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of...
Ausführliche Beschreibung
Autor*in: |
Bush, R. I. [verfasserIn] Scheick, X. [verfasserIn] Scherrer, P. [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
s.l.: Macmillan Magazines Ltd. ; 1998 |
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Umfang: |
3 |
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Reproduktion: |
Nature Archives 1869 - 2009 |
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Übergeordnetes Werk: |
In: Nature |
Übergeordnetes Werk: |
volume:392 ; year:1998 ; number:6672 ; month:01 ; pages:155-157 ; extent:3 |
Links: |
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DOI / URN: |
10.1038/32361 |
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10.1038/32361 doi (DE-627)NLEJ234967390 DE-627 ger DE-627 rakwb eng Bush, R. I. verfasserin aut The Sun's shape and brightness [s.l.] Macmillan Magazines Ltd. 1998 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... Nature Archives 1869 - 2009 Scheick, X. verfasserin aut Scherrer, P. verfasserin aut Kuhn, J. R. oth In Nature <London> London [u.a.] : Nature Publising Group, 1869 392(1998), 6672 vom: Jan., Seite 155-157 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:392 year:1998 number:6672 month:01 pages:155-157 extent:3 http://dx.doi.org/10.1038/32361 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 392 1998 6672 1 155-157 3 |
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10.1038/32361 doi (DE-627)NLEJ234967390 DE-627 ger DE-627 rakwb eng Bush, R. I. verfasserin aut The Sun's shape and brightness [s.l.] Macmillan Magazines Ltd. 1998 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... Nature Archives 1869 - 2009 Scheick, X. verfasserin aut Scherrer, P. verfasserin aut Kuhn, J. R. oth In Nature <London> London [u.a.] : Nature Publising Group, 1869 392(1998), 6672 vom: Jan., Seite 155-157 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:392 year:1998 number:6672 month:01 pages:155-157 extent:3 http://dx.doi.org/10.1038/32361 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 392 1998 6672 1 155-157 3 |
allfields_unstemmed |
10.1038/32361 doi (DE-627)NLEJ234967390 DE-627 ger DE-627 rakwb eng Bush, R. I. verfasserin aut The Sun's shape and brightness [s.l.] Macmillan Magazines Ltd. 1998 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... Nature Archives 1869 - 2009 Scheick, X. verfasserin aut Scherrer, P. verfasserin aut Kuhn, J. R. oth In Nature <London> London [u.a.] : Nature Publising Group, 1869 392(1998), 6672 vom: Jan., Seite 155-157 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:392 year:1998 number:6672 month:01 pages:155-157 extent:3 http://dx.doi.org/10.1038/32361 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 392 1998 6672 1 155-157 3 |
allfieldsGer |
10.1038/32361 doi (DE-627)NLEJ234967390 DE-627 ger DE-627 rakwb eng Bush, R. I. verfasserin aut The Sun's shape and brightness [s.l.] Macmillan Magazines Ltd. 1998 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... Nature Archives 1869 - 2009 Scheick, X. verfasserin aut Scherrer, P. verfasserin aut Kuhn, J. R. oth In Nature <London> London [u.a.] : Nature Publising Group, 1869 392(1998), 6672 vom: Jan., Seite 155-157 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:392 year:1998 number:6672 month:01 pages:155-157 extent:3 http://dx.doi.org/10.1038/32361 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 392 1998 6672 1 155-157 3 |
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10.1038/32361 doi (DE-627)NLEJ234967390 DE-627 ger DE-627 rakwb eng Bush, R. I. verfasserin aut The Sun's shape and brightness [s.l.] Macmillan Magazines Ltd. 1998 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... Nature Archives 1869 - 2009 Scheick, X. verfasserin aut Scherrer, P. verfasserin aut Kuhn, J. R. oth In Nature <London> London [u.a.] : Nature Publising Group, 1869 392(1998), 6672 vom: Jan., Seite 155-157 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:392 year:1998 number:6672 month:01 pages:155-157 extent:3 http://dx.doi.org/10.1038/32361 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 392 1998 6672 1 155-157 3 |
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[Auszug] The origin of the 11- and 22-year solar cycles remains one of the more mysterious aspects of the Sun. These cycles are probably driven by convection in the solar interior, but the convection zone is difficult to probe. Small departures from sphericity in the effective surface temperature of the ... |
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